Year: 2025
Type: article
Abstract: GeV gamma-ray emission is frequently observed both at large angular separation from pulsars and are not always centered around these pulsars. Using GPU-acceleration monte-carlo simulations, the authors provide a compelling explanation that the propogation of 100 GeV electrons that produce these gamma-rays in the turbulent interstellar magnetic field both leads to off-center peaks and wide separation, e.g., a gamma-ray mirage. These mirages can help constrain the properties of the interstellar magnetic field.
DOI: 10.1103/9461-gltv
Institutions: Shanghai Jiao Tong University, Nanjing University
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W4417065350
